Gravity Acceleration Equation:
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Gravity acceleration (g) is the acceleration experienced by an object due to the gravitational force of a massive body. It describes how quickly an object's velocity changes when falling freely under gravity's influence.
The calculator uses the universal gravity acceleration equation:
Where:
Explanation: This formula calculates the gravitational acceleration at a specific distance from a massive object's center, based on Newton's law of universal gravitation.
Details: Calculating gravity acceleration is essential for space missions, satellite orbits, planetary science, and understanding fundamental physics principles. It helps determine orbital velocities, escape velocities, and gravitational forces.
Tips: Enter the gravitational constant (pre-filled with standard value), mass of the celestial body in kilograms, and distance from center in meters. All values must be positive numbers.
Q1: What is Earth's gravity acceleration at surface?
A: Approximately 9.8 m/s², calculated using Earth's mass (5.972 × 10²⁴ kg) and radius (6.371 × 10⁶ m).
Q2: Why does gravity decrease with distance?
A: Gravity follows an inverse-square law - doubling the distance reduces gravity to one-quarter of its original strength.
Q3: What is the gravitational constant value?
A: G = 6.67430 × 10⁻¹¹ m³ kg⁻¹ s⁻², one of the fundamental constants of nature.
Q4: How does mass affect gravity acceleration?
A: Greater mass produces stronger gravitational acceleration, as g is directly proportional to mass M.
Q5: Can this calculate gravity on other planets?
A: Yes, simply input the planet's mass and radius to calculate surface gravity for any celestial body.